Cassini UVIS observatory phase spectral imaging of the Saturn system D. Shemansky(1) Cassini UVIS team(2 – 6) PI: L. Esposito (1)University of Southern California, (2) University of Colorado, Boulder, (3)Max Planck Inst (MPIS), (4)JPL, (5) C. Az. Coll., (6)Calif. Inst. Technology History of neutral gas measurements and analysis • Atomic hydrogen predicted by McDonough and Brice (1973) as a torus at Titan orbit • Detected by Weiser et al. (1975) with JHU rocket. Undetermined location, but assumed to be at Titan orbit. • Voyager UVS: Broadfoot et al. (1977). Interpreted as a torus. •Sittler et al. (1981): Report energetic electron depletion in 2.8 RS to 3.7 RS region and infer possible neutral gas as absorber. Identify separate absorption effect of a larger E-ring presence. •Hood (1989): Found large losses of energetic protons in the 5 to 12 RS region inadequately explained by then known gas abundances or ring particles. •Shemansky and Hall (1992): Analyzed Voyager 1 data, concluding that the entire magnetosphere is filled with atomic hydrogen merging into the top of the Saturn atmosphere. Energy sink analysis of the very low electron temperature in the plasma sheet reported by the PLS experiment is used to predict large abundance of the neutral oxygen and hydroxyl radical water dissociation products. S&H(1992) Voyager 1 Saturn atomic hydrogen Cassini UVIS image of atomic hydrogen in the Saturn system Cassini UVIS image of atomic hydrogen in the Saturn system History continued • OH discovered in the 3 – 6 RS region of the Saturn magnetosphere using HST [Shemansky et al., 1993] • OI discovered using Cassini UVIS imaging, Dec 25, 2003 – May 13, 2004. Simulation of core neutral gas distribution OH (from HST) vs OI torus OH OI Total neutral gas abundance • atomic hydrogen: 2 X 1035 atoms Loss rate: > 1.3 X 1027 atoms s-1 • atomic oxygen: 3 – 4 X 1034 atoms Loss rate: ~ 1028 atoms s-1 Characteristics of UVIS observations • The abundance of OI increased from Dec/Jan to a peak in Feb/March and declined to slightly less than the original value by mid May. • The OI distribution in the orbital plane expanded outward in Feb/March and contracted inward in following months. • The peak emission shows a distinct asymmetry in the early months, peaking on the planet darkside. Implications of UVIS observations • The rise and fall in abundance of OI between Dec 25, 2003 and May 13, 2004 amounts to at total inferred ~500 Mkg of mass apparently lost from the system in this period. Mean loss rate of bulge in mass during 2 months is ~4 X 1027 atoms s-1. • Total mass of OI + OH in system is ~2200. Mkg. • The estimated mass of micron sized particles in the E-ring involved in the Mimas – Tethys region is 600 Mkg. Implications continued • Using the plasma sheet model (Richardson, 1997) based on the Voyager PLS measurements, the charge capture characteristic time for loss of OI is 40 days. This independent rate process loss rate also indicates that mass equal to the micron sized E-ring particles is lost from Saturn in 1 to 2 months. • Including the projected unobserved ~5 km E-ring objects, the lifetime of the entire Ering against this process is ~100 M years. Proposed primary water product plasma reactions: Neutral gas loss processes: O + O+ O+ + O OH + O+ OH+ + O H+ + O O+ + H O+ + H H+ + O Reactions continued Neutral Gas production: Plasma loss: Cluster-ion formation O2H2+.(H2O)n.G + e O2 + H2 + G O2H2+.(H2O)n.G + e O + H + OH + G O2H2+.(H2O)n.G + e O2 + H + H + G H3O+. (H2O)n.G + e OH + H2 + G H3O+.(H2O)n.G + e O + 3H + G Neutral and plasma loss OH+ + e O + H Conclusions • The UVIS imaging of the OI population in the magnetosphere has revealed a very complex system that is eroding icy solids at a high rate. The required large exposed surface area implies micron and smaller particles are the primary reaction targets. • We propose that low energy plasma ions forming solid state cluster ions may be the primary neutral gas source process and plasma quenching reaction. • A single stochastic event has been observed, that may represent one erosion mechanism. Conclusions continued • The required energy deposition for the erosion process (~14gW) is plausibly moderately energetic magnetospheric electrons, that derive their energy from the rotating magnetic field. • The Saturn magnetosphere is completely different from that of Jupiter. Jupiter neutral/ion = ~0.003 Saturn neutral/ion = ~100.